Neutrinos from SN1987a in the IMB detector
Neutrinos from SN1987a in the IMB detector
复制标题
IMB 探测器中来自 SN1987a 的中微子
DOI：
10.1016/0168-9002(88)91097-2
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发表时间：
1988
影响因子：
1.4
通讯作者：
J. Velde
中科院分区：
文献类型：
--
作者：
T. Haines;C. B. Bratton;D. Casper;A. Ciocio;R. Claus;M. Crouch;S. Dye;S. Errede;W. Gajewski;M. Goldhaber;T. Jones;D. Kiełczewska;W. Kropp;J. Learned;J. LoSecco;J. Matthews;R. Miller;M. Mudan;L. Price;F. Reines;J. Schultz;S. Seidel;E. Shumard;D. Sinclair;H. Sobel;L. Sulak;R. Svoboda;G. Thornton;J. Velde
IMB 探测器观测到在大麦哲伦星云中的超新星光学探测之前爆发的八个中微子事件。这些事件的间隔为 6 秒，可见能量范围为 20-40 MeV。对信号与超新星的预期信号进行了一些比较。在 IMB 运行期间，我们没有发现其他类似的爆发。
A burst of eight neutrino events preceding the optical detection of the supernova in the Large Magellanic Cloud has been observed by the IMB detector. The events span an interval of 6 s and have visible energies in the range 20–40 MeV. Some comparisons between the signal and that expected from a supernova are made. We have found no other comparable burst during the operation of IMB.